Black holes in anti-de Sitter: quasinormal modes, tails and tales of flat spacetime

Abstract

Black holes in asymptotically anti-de Sitter (AdS) spacetimes have been the subject of intense scrutiny, including detailed frequency-domain analysis and full nonlinear evolutions. Remarkably, studies of linearized perturbations in the time-domain are scarce or non-existing. We close this gap by evolving linearized scalar wavepackets in the background of rotating BHs in AdS spacetimes. Our results show a number of interesting features. Small BHs in AdS behave as asymptotically flat BHs for early/intermediate times, displaying the same ringdown modes and power-law tails. As the field bounces back and forth between the horizon and the timelike boundary it "thermalizes" and the modes of AdS settle in. Finally, we have indications that wavepackets in the vicinity of fastly spinning BHs grow exponentially in time, signalling a superradiant instability of the geometry previously reported through a frequency-domain analysis.

6 pages, RevTex4. Accepted for publication in Physical Review D. v2: References added

References in corpus (6)

• Minkowski-space correlators in AdS/CFT correspondence: recipe and applications
• Can environmental effects spoil precision gravitational-wave astrophysics?
• Quasinormal ringing of Kerr black holes: The excitation factors
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Cited by in corpus (2)

• Structural aspects of the anti-de Sitter black hole pseudospectrum
• Quasinormal modes of anyons